CWNU 1347

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0.43 UTI
0.47
CN
0.69
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 5.2 [arcmin]
  • CN 0.47 Poorly populated
  • Cdens 0.69 Moderately dense
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1347 is a poorly populated, moderately dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.
Relatively close High extinction Massive Near-solar metallicity Young

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 257.464 -40.482 0.411 -1.188 -2.337 -2.113
Hunt & Reffert 2024 257.467 -40.49 0.402 -1.201 -2.396 -3.64
Cavallo et al. 2024 257.428 -40.519 0.402 – – –
Hunt & Reffert 2023 257.467 -40.49 0.402 -1.201 -2.396 -3.64
He et al. 2023 257.471 -40.491 0.414 -1.174 -2.324 -0.98

💡 Note: The UCC values are estimated from its identified members.

Reference Year Dist [kpc] Av [mag] DAv [mag] Age [Myr] [Fe/H] [dex] Mass [Msun] Bfr BSS
Hunt & Reffert 2024 – – – – – 1305* – –
Cavallo et al. 2024 2.30 4.89 – 87 0.330 – – –
Hunt & Reffert 2023 2.28 4.77 2.82 177 – – – –
He et al. 2023 2.63 5.45 – 1 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

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